Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S
Context. To study the evolution of Li in the Galaxy it is necessary to observe dwarf or subgiant stars. These are the only long-lived stars whose present-day atmospheric chemical composition reflects their natal Li abundances according to standard models
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